Studying the atmosphere of HD 189733 b using the Rossiter-McLaughlin effect

Thesis: S.B., Massachusetts Institute of Technology, Department of Earth, Atmospheric, and Planetary Sciences, May, 2020

Bibliographic Details
Main Author: Minsky, Charlotte(Charlotte L.)
Other Authors: Richard P. Binzel.
Format: Thesis
Language:eng
Published: Massachusetts Institute of Technology 2021
Subjects:
Online Access:https://hdl.handle.net/1721.1/130194
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author Minsky, Charlotte(Charlotte L.)
author2 Richard P. Binzel.
author_facet Richard P. Binzel.
Minsky, Charlotte(Charlotte L.)
author_sort Minsky, Charlotte(Charlotte L.)
collection MIT
description Thesis: S.B., Massachusetts Institute of Technology, Department of Earth, Atmospheric, and Planetary Sciences, May, 2020
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spelling mit-1721.1/1301942021-03-23T03:21:31Z Studying the atmosphere of HD 189733 b using the Rossiter-McLaughlin effect Minsky, Charlotte(Charlotte L.) Richard P. Binzel. Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences. Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences Earth, Atmospheric, and Planetary Sciences. Thesis: S.B., Massachusetts Institute of Technology, Department of Earth, Atmospheric, and Planetary Sciences, May, 2020 Cataloged from student-submitted PDF of thesis. "May 21 2019." Includes bibliographical references (pages 29-32). Transmission spectroscopy is a widely-used method for studying exoplanetary atmospheres. However, the differential data analysis techniques that are generally applied to high-resolution ground-based spectroscopic data are only sensitive to narrow spectral features and do not preserve broadband features. This makes them insensitive to the strong Rayleigh scattering slope of HD 189733 b that is due to possible atmospheric aerosols. The Rossiter-McLaughlin (RM) effect provides a way to probe broadband spectral features because its amplitude varies as a function of wavelength according to the effective planet radius. Previously, radial velocity (RV) variations caused by the RM effect were interpreted as being a tentative detection (2.5[sigma]) of the broadband scattering slope of HD 189733 b. We developed a new method that directly models the distortions in spectral lines (rather than the resulting RV variation) and applied this method to the same archival HARPS data that was used in the previous tentative detection. Here we will present this method and the ongoing work necessarily to problem-solve and fully implement it. by Charlotte Minsky. S.B. S.B. Massachusetts Institute of Technology, Department of Earth, Atmospheric, and Planetary Sciences 2021-03-22T17:12:59Z 2021-03-22T17:12:59Z 2019 2020 Thesis https://hdl.handle.net/1721.1/130194 1241180991 eng MIT theses may be protected by copyright. Please reuse MIT thesis content according to the MIT Libraries Permissions Policy, which is available through the URL provided. http://dspace.mit.edu/handle/1721.1/7582 32 pages application/pdf Massachusetts Institute of Technology
spellingShingle Earth, Atmospheric, and Planetary Sciences.
Minsky, Charlotte(Charlotte L.)
Studying the atmosphere of HD 189733 b using the Rossiter-McLaughlin effect
title Studying the atmosphere of HD 189733 b using the Rossiter-McLaughlin effect
title_full Studying the atmosphere of HD 189733 b using the Rossiter-McLaughlin effect
title_fullStr Studying the atmosphere of HD 189733 b using the Rossiter-McLaughlin effect
title_full_unstemmed Studying the atmosphere of HD 189733 b using the Rossiter-McLaughlin effect
title_short Studying the atmosphere of HD 189733 b using the Rossiter-McLaughlin effect
title_sort studying the atmosphere of hd 189733 b using the rossiter mclaughlin effect
topic Earth, Atmospheric, and Planetary Sciences.
url https://hdl.handle.net/1721.1/130194
work_keys_str_mv AT minskycharlottecharlottel studyingtheatmosphereofhd189733busingtherossitermclaughlineffect